Critical gravitational collapse with angular momentum
arXiv:1608.00491 · doi:10.1103/PhysRevD.94.084012
Abstract
We derive a theoretical model of mass and angular momentum scaling in type-II critical collapse with rotation. We focus on the case where the critical solution has precisely one, spherically symmetric, unstable mode. We demonstrate excellent agreement with numerical results for critical collapse of a rotating radiation fluid, which falls into this case.
Version accepted for publication in PRD
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- Critical phenomena in the gravitational collapse of electromagnetic waves
- Aspherical deformations of the Choptuik spacetime
- Critical behavior in 3-d gravitational collapse of massless scalar fields
- Critical phenomena in gravitational collapse with two competing massless matter fields
- Critical gravitational collapse with angular momentum II: soft equations of state
- Non-spherical effects on the mass function of Primordial Black Holes
- Critical collapse of ultra-relativistic fluids: damping or growth of aspherical deformations
- Simulations of Ellipsoidal Primordial Black Hole Formation
- Effective inspiral spin distribution of primordial black hole binaries
- Twist and higher modes of a complex scalar field at the threshold of collapse